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Michelle Harris - One of the best experts on this subject based on the ideXlab platform.
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Integrated Ocean Drilling Program Expedition 335 Preliminary Report: Superfast Spreading Rate Crust 4. Drilling gabbro in intact ocean crust formed at a superfast spreading rate, 13 April–3 June 2011
2020Co-Authors: Damon A. H. Teagle, Expedition Scientists, Michelle HarrisAbstract:The Superfast Spreading Crust campaign, echoing long-standing ocean lithosphere community endeavors, was designed to help us understand the formation, architecture, and evolution of ocean crust formed at fast spreading rates. Integrated Ocean Drilling Program (IODP) Expedition 335, “Superfast Spreading Rate Crust 4” (13 April–3 June 2011), was the fourth scientific drilling cruise of the Superfast Spreading Crust campaign to Ocean Drilling Program (ODP) Hole 1256D. The expedition aimed to deepen this basement reference site several hundred meters into the gabbroic rocks of intact lower oceanic crust to address the following fundamental scientific questions: Does the lower crust form by subsidence of a crystal mush from a high-level magma chamber (gabbro glacier), by intrusion of sills throughout the lower crust, or by some other mechanism? How does melt percolate through the lower crust, and what are the reactions and chemical evolution of magmas during migration? Is the plutonic crust cooled by conduction or hydrothermal circulation? What are the role and extent of deeply penetrating seawater-derived hydrothermal fluids in cooling the lower crust and the chemical exchanges between the ocean crust and the oceans? What are the relationships among the geological, geochemical, and geophysical structure of the crust and, in particular, the nature of the seismic Layer 2–3 transition? What is the magnetic contribution of the lower crust to marine magnetic anomalies? Hole 1256D is located on 15 Ma crust in the eastern equatorial Pacific Ocean (6°44.163?N, 91°56.061?W). Oceanic crust that formed at a superfast spreading rate (>200 mm/y) was specifically targeted to exploit the observed relationship between spreading rate and depth to axial low-velocity zones, thought to be magma chambers, seismically imaged at active mid-ocean ridges. This was a deliberate strategy to reduce the drilling distance to gabbroic rocks because thick sequences of lavas and dikes have proved difficult to penetrate in the past. Previous cruises to ODP Site 1256 (ODP Leg 206; IODP Expedition 309/312) have achieved their leg- and expedition-specific objectives but not the overarching strategic goals of the Superfast Spreading Crust campaign to understand magmatic accretion at fast-spreading ocean ridges. However, the three previous cruises achieved the first complete sampling of intact upper oceanic crust and successfully drilled through ~800 m of erupted lavas and thin (~345 m) sheeted dike complex and sampled gabbros at ~1157 meters subbasement. The lowermost 100 m of the hole is a complex dike–plutonic transition zone and comprises two gabbro lenses intruded into very strongly contact metamorphosed, granoblastically recrystallized sheeted dikes. During Expedition 335, we reentered Hole 1256D more than 5 years after our last visit and encountered and overcame a number of significant engineering challenges, each unique but of natures not unexpected in a deep, uncased marine borehole into igneous rocks. The patient, persistent efforts of the Rig Floor teams cleared a major obstruction at 920 meters below seaFloor (mbsf) that initially prevented reentry into the hole to its full depth (1507 mbsf). The 920–960 mbsf interval was then cemented to stabilize the borehole wall. A short phase of coring deepened Hole 1256D ~13 m before the C-9 hard formation coring bit failed and was ground to a smooth stump. A progressive, logical course of action was then undertaken to clear the bottom of the hole of metal junk from the failed coring bit, open up a short interval of undergauge hole, and remove a very large amount of drilling cuttings from the hole. This was successfully completed, and the hole is open to its full depth (1521.6 mbsf). The hole-cleaning phase was followed by wireline caliper and temperature measurements of the complete hole to assist with cementing operations to stabilize the lowermost 10 m of the hole and the problematic interval at 910–940 mbsf. These remedial efforts should facilitate reentry and coring on a future return to Hole 1256D. In addition to the few cores drilled, the junk baskets deployed during the successive fishing runs to the bottom of the hole recovered a unique collection of samples, including large cobbles (as large as 5 kg), angular rubble, and fine cuttings of principally strongly to completely recrystallized granoblastic basalt with minor gabbroic rocks and evolved plutonic rocks. The large blocks exhibit intrusive, structural, and textural relationships, along with overprinting and crosscutting hydrothermal alteration and metamorphic paragenetic sequences that hitherto have not been observed because of the small diameter of drill cores and the very low recovery of the granoblastic dikes cored so far. The high extent of metamorphic recrystallization exhibited by the granoblastic basalt, combined with operational factors, provides strong evidence that most of this material comes from the lowermost reaches of Hole 1256D (~1495 to ~1522 mbsf). Including the ~60 m thick zone of granoblastic dikes that reside above the uppermost gabbros, the dike–gabbro transition zone at Site 1256 is >170 m thick, of which >100 m is recrystallized granoblastic basalt. When the textural and contact relationships exhibited by these samples are placed in the geological context of the Hole 1256D stratigraphy, a vision emerges of a complex, dynamic thermal boundary layer zone. This region of the crust between the principally hydrothermal domain of the upper crust and the intrusive magmatic domain of the lower crust is one of evolving geological conditions. An intimate coupling among temporally and spatially intercalated magmatic, hydrothermal, partial melting, intrusive, metamorphic, and retrograde processes is recorded in the recovered samples. Expedition 335 left Hole 1256D after making only a very modest advance, and we have yet to recover the samples of cumulate gabbros required to test models of ocean ridge magmatic accretion and the intensity of hydrothermal cooling at depth. However, a remarkable sample suite of granoblastic basalt with minor gabbros, some of which intrude previously recrystallized dikes, was recovered and provides a detailed picture of a rarely sampled critical interval of the oceanic crust. Most importantly, the hole has been stabilized, cleared to its full depth, and is ready for deepening in the near future.
Ugochukwu Nnamdi Okafor - One of the best experts on this subject based on the ideXlab platform.
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Evaluation of liquid lift approach to dual gradient drilling
2008Co-Authors: Ugochukwu Nnamdi OkaforAbstract:Evaluation of Liquid Lift Approach to Dual Gradient Drilling. (December 2007) Ugochukwu Nnamdi Okafor, B.S., University of Lagos, Nigeria Chair of Advisory Committee: Dr. Hans C. Juvkam-Wold In the past, the oil and gas industry has typically used the single gradient system to drill wells offshore. With this system the bottom hole pressure was controlled by a mud column extending from the drilling Rig to the bottom of the wellbore. This mud column was used to achieve the required bottom hole pressure. But, as the demand for oil and gas increased, the industry started exploring for oil and gas in deep waters. Because of the narrow margin between the pore and fracture pressures it is somewhat difficult to reach total depth with the single gradient system. This led to the invention of the dual gradient system. In the dual gradient method, heavy density fluid runs from the bottom hole to the mudline and a low density fluid from the mudline to the Rig Floor so as to maintain the bottom hole pressure. Several methods have been developed to achieve the dual gradient drilling principle. For this research project, we paid more attention to the liquid lift, dual gradient drilling (riser dilution method). This method of achieving dual gradient drilling was somewhat different from the others, because it does not utilize elaborate equipment and no major changes are made on the existing drilling Rigs.
Damon A. H. Teagle - One of the best experts on this subject based on the ideXlab platform.
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Integrated Ocean Drilling Program Expedition 335 Preliminary Report: Superfast Spreading Rate Crust 4. Drilling gabbro in intact ocean crust formed at a superfast spreading rate, 13 April–3 June 2011
2020Co-Authors: Damon A. H. Teagle, Expedition Scientists, Michelle HarrisAbstract:The Superfast Spreading Crust campaign, echoing long-standing ocean lithosphere community endeavors, was designed to help us understand the formation, architecture, and evolution of ocean crust formed at fast spreading rates. Integrated Ocean Drilling Program (IODP) Expedition 335, “Superfast Spreading Rate Crust 4” (13 April–3 June 2011), was the fourth scientific drilling cruise of the Superfast Spreading Crust campaign to Ocean Drilling Program (ODP) Hole 1256D. The expedition aimed to deepen this basement reference site several hundred meters into the gabbroic rocks of intact lower oceanic crust to address the following fundamental scientific questions: Does the lower crust form by subsidence of a crystal mush from a high-level magma chamber (gabbro glacier), by intrusion of sills throughout the lower crust, or by some other mechanism? How does melt percolate through the lower crust, and what are the reactions and chemical evolution of magmas during migration? Is the plutonic crust cooled by conduction or hydrothermal circulation? What are the role and extent of deeply penetrating seawater-derived hydrothermal fluids in cooling the lower crust and the chemical exchanges between the ocean crust and the oceans? What are the relationships among the geological, geochemical, and geophysical structure of the crust and, in particular, the nature of the seismic Layer 2–3 transition? What is the magnetic contribution of the lower crust to marine magnetic anomalies? Hole 1256D is located on 15 Ma crust in the eastern equatorial Pacific Ocean (6°44.163?N, 91°56.061?W). Oceanic crust that formed at a superfast spreading rate (>200 mm/y) was specifically targeted to exploit the observed relationship between spreading rate and depth to axial low-velocity zones, thought to be magma chambers, seismically imaged at active mid-ocean ridges. This was a deliberate strategy to reduce the drilling distance to gabbroic rocks because thick sequences of lavas and dikes have proved difficult to penetrate in the past. Previous cruises to ODP Site 1256 (ODP Leg 206; IODP Expedition 309/312) have achieved their leg- and expedition-specific objectives but not the overarching strategic goals of the Superfast Spreading Crust campaign to understand magmatic accretion at fast-spreading ocean ridges. However, the three previous cruises achieved the first complete sampling of intact upper oceanic crust and successfully drilled through ~800 m of erupted lavas and thin (~345 m) sheeted dike complex and sampled gabbros at ~1157 meters subbasement. The lowermost 100 m of the hole is a complex dike–plutonic transition zone and comprises two gabbro lenses intruded into very strongly contact metamorphosed, granoblastically recrystallized sheeted dikes. During Expedition 335, we reentered Hole 1256D more than 5 years after our last visit and encountered and overcame a number of significant engineering challenges, each unique but of natures not unexpected in a deep, uncased marine borehole into igneous rocks. The patient, persistent efforts of the Rig Floor teams cleared a major obstruction at 920 meters below seaFloor (mbsf) that initially prevented reentry into the hole to its full depth (1507 mbsf). The 920–960 mbsf interval was then cemented to stabilize the borehole wall. A short phase of coring deepened Hole 1256D ~13 m before the C-9 hard formation coring bit failed and was ground to a smooth stump. A progressive, logical course of action was then undertaken to clear the bottom of the hole of metal junk from the failed coring bit, open up a short interval of undergauge hole, and remove a very large amount of drilling cuttings from the hole. This was successfully completed, and the hole is open to its full depth (1521.6 mbsf). The hole-cleaning phase was followed by wireline caliper and temperature measurements of the complete hole to assist with cementing operations to stabilize the lowermost 10 m of the hole and the problematic interval at 910–940 mbsf. These remedial efforts should facilitate reentry and coring on a future return to Hole 1256D. In addition to the few cores drilled, the junk baskets deployed during the successive fishing runs to the bottom of the hole recovered a unique collection of samples, including large cobbles (as large as 5 kg), angular rubble, and fine cuttings of principally strongly to completely recrystallized granoblastic basalt with minor gabbroic rocks and evolved plutonic rocks. The large blocks exhibit intrusive, structural, and textural relationships, along with overprinting and crosscutting hydrothermal alteration and metamorphic paragenetic sequences that hitherto have not been observed because of the small diameter of drill cores and the very low recovery of the granoblastic dikes cored so far. The high extent of metamorphic recrystallization exhibited by the granoblastic basalt, combined with operational factors, provides strong evidence that most of this material comes from the lowermost reaches of Hole 1256D (~1495 to ~1522 mbsf). Including the ~60 m thick zone of granoblastic dikes that reside above the uppermost gabbros, the dike–gabbro transition zone at Site 1256 is >170 m thick, of which >100 m is recrystallized granoblastic basalt. When the textural and contact relationships exhibited by these samples are placed in the geological context of the Hole 1256D stratigraphy, a vision emerges of a complex, dynamic thermal boundary layer zone. This region of the crust between the principally hydrothermal domain of the upper crust and the intrusive magmatic domain of the lower crust is one of evolving geological conditions. An intimate coupling among temporally and spatially intercalated magmatic, hydrothermal, partial melting, intrusive, metamorphic, and retrograde processes is recorded in the recovered samples. Expedition 335 left Hole 1256D after making only a very modest advance, and we have yet to recover the samples of cumulate gabbros required to test models of ocean ridge magmatic accretion and the intensity of hydrothermal cooling at depth. However, a remarkable sample suite of granoblastic basalt with minor gabbros, some of which intrude previously recrystallized dikes, was recovered and provides a detailed picture of a rarely sampled critical interval of the oceanic crust. Most importantly, the hole has been stabilized, cleared to its full depth, and is ready for deepening in the near future.
J.a. Burton - One of the best experts on this subject based on the ideXlab platform.
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Real-time feedback for subsea casing-hanger landing operations
2020Co-Authors: T. J. Allen, J.a. Burton, M. T. Worsley, K. W. ElliotAbstract:An intelligent running tool, a smart tool, for subsea casing-hanger landing operations provides feedback of critical parameters while landing and cementing the casing and while setting and testing the casing-hanger seal assembly subsea. Two-way communication between the Rig Floor and the running tool in the subsea wellhead provides real-time data to make quick informed decisions regarding operations. The information provides positive feedback of the casing-hanger position and status of the seal assembly.
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Intelligent Running Tools for Subsea Drilling and Completion Equipment Using Acoustical Two-Way Communication Between the Subsea Wellhead and the Surface
Offshore Technology Conference, 1990Co-Authors: J.a. Burton, T.g. Cassity, B.m. Taylor, J.d. MartinAbstract:The development of intelligent running tools (smart tools) for subsea drilling and completion equipment is presented. The system provides intelligent feedback of critical parameters while landing and operating subsea marine wellhead equipment. Two way communication is provided between the Rig Floor and the subsea wellhead, and real time data is provided to the operator to allow informed decisions to be quickly made. Many other subsea applications are envisioned for this simple and rugged communication system.
J. C. Eggemeyer - One of the best experts on this subject based on the ideXlab platform.
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Field test of a full-scale dual-gradient drilling system
2020Co-Authors: J. P. Schumacher, J. D. Dowell, L. R. Ribbeck, J. C. EggemeyerAbstract:Dual-gradient drilling (DGD) provides the same bottomhole pressure as a single mud weight from the surface to total depth (TD) with a combination of two fluid gradients: slightly heavier mud from the mudline to TD and seawater from the mudline back up to the Rig Floor. With DGD, margins between fracture gradient and pore pressure are significantly greater while drilling the well. Lower-cost wells can be drilled by use of DGD more safely and with more completion flexibility than with single-gradient systems.
